The Cosmic Neutrino Background Anisotropy - Linear Theory - Astrophysics > Cosmology and Nongalactic AstrophysicsReportar como inadecuado




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Abstract: The cosmic neutrino background anisotropy is calculated for massive neutrinostates by solving the full Boltzmann equation. The effect of weak gravitationallensing, including the Limber approximation, is also derived for massiveparticles, and subsequently applied to the case of massive neutrinos.



Autor: Steen Hannestad, Jacob Brandbyge University of Aarhus

Fuente: https://arxiv.org/







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